D-Index & Metrics Best Publications

D-Index & Metrics D-index (Discipline H-index) only includes papers and citation values for an examined discipline in contrast to General H-index which accounts for publications across all disciplines.

Discipline name D-index D-index (Discipline H-index) only includes papers and citation values for an examined discipline in contrast to General H-index which accounts for publications across all disciplines. Citations Publications World Ranking National Ranking
Physics D-index 70 Citations 21,573 290 World Ranking 3059 National Ranking 58

Overview

What is she best known for?

The fields of study she is best known for:

  • Galaxy
  • Astronomy
  • Astrophysics

Her primary areas of study are Astrophysics, Galaxy, Astronomy, Stellar population and Metallicity. Her Astrophysics research includes elements of Spectral line and Spectral resolution. Galaxy connects with themes related to Starlight in her study.

Her Surface brightness, Galaxy cluster, Disc and Bulge study in the realm of Astronomy connects with subjects such as Christian ministry. As part of one scientific family, Patricia Sanchez-Blazquez deals mainly with the area of Stellar population, narrowing it down to issues related to the Radius, and often Morphological type and Critical value. Her work deals with themes such as Spiral galaxy and Velocity dispersion, which intersect with Metallicity.

Her most cited work include:

  • Medium-resolution isaac newton telescope library of empirical spectra (1127 citations)
  • Medium-resolution isaac newton telescope library of empirical spectra (1127 citations)
  • Medium-resolution isaac newton telescope library of empirical spectra (1127 citations)

What are the main themes of her work throughout her whole career to date?

Her primary scientific interests are in Astrophysics, Galaxy, Astronomy, Star formation and Stellar population. Metallicity, Elliptical galaxy, Stars, Velocity dispersion and Galaxy formation and evolution are among the areas of Astrophysics where the researcher is concentrating her efforts. Her Stars research integrates issues from Interstellar medium and Supernova.

Galaxy is closely attributed to Spectral line in her work. Her Star formation study combines topics in areas such as Luminosity, Radius and Effective radius. Her Stellar population study deals with Spectral resolution intersecting with Telescope.

She most often published in these fields:

  • Astrophysics (118.50%)
  • Galaxy (87.82%)
  • Astronomy (63.70%)

What were the highlights of her more recent work (between 2017-2021)?

  • Astrophysics (118.50%)
  • Galaxy (87.82%)
  • Star formation (41.45%)

In recent papers she was focusing on the following fields of study:

Her primary areas of study are Astrophysics, Galaxy, Star formation, Metallicity and Stellar population. Her Astrophysics study frequently draws parallels with other fields, such as Radius. As part of her studies on Galaxy, Patricia Sanchez-Blazquez frequently links adjacent subjects like Stars.

The study incorporates disciplines such as Local Group, Dwarf galaxy, Galaxy formation and evolution and Spatially resolved in addition to Star formation. Her Metallicity research focuses on Line and how it relates to Interstellar medium. Patricia Sanchez-Blazquez has researched Stellar population in several fields, including Extinction, Spectral energy distribution and Universe.

Between 2017 and 2021, her most popular works were:

  • J-PLUS: The Javalambre Photometric Local Universe Survey. (58 citations)
  • J-PLUS: The Javalambre Photometric Local Universe Survey (51 citations)
  • Time Inference with MUSE in Extragalactic Rings (TIMER): properties of the survey and high-level data products (50 citations)

In her most recent research, the most cited papers focused on:

  • Galaxy
  • Astronomy
  • Astrophysics

Her main research concerns Astrophysics, Galaxy, Stellar population, Star formation and Metallicity. Astrophysics and Radius are commonly linked in her work. Her work on Secular evolution, Spiral galaxy, Redshift and Luminosity as part of general Galaxy study is frequently connected to Bar, therefore bridging the gap between diverse disciplines of science and establishing a new relationship between them.

Stellar population and Universe are frequently intertwined in her study. Her Star formation research focuses on Velocity dispersion and how it connects with Star cluster. The various areas that Patricia Sanchez-Blazquez examines in her Metallicity study include Large Magellanic Cloud and Local Group, Leo A, Dwarf galaxy.

This overview was generated by a machine learning system which analysed the scientist’s body of work. If you have any feedback, you can contact us here.

Best Publications

MILES: A Medium resolution INT Library of Empirical Spectra

Patricia Sanchez-Blazquez;Reynier Peletier;Jorge Jimenez-Vicente;Nicolas Cardiel.
arXiv: Astrophysics (2006)

1892 Citations

Medium-resolution isaac newton telescope library of empirical spectra

P. Sanchez-Blazquez;P. Sanchez-Blazquez;P. Sanchez-Blazquez;R. F. Peletier;R. F. Peletier;J. Jimenez-Vicente;N. Cardiel.
Monthly Notices of the Royal Astronomical Society (2006)

1373 Citations

CALIFA, the Calar Alto Legacy Integral Field Area survey : I. Survey presentation

S. F. Sánchez;R. C. Kennicutt;A. Gil de Paz;G. van de Ven.
Astronomy and Astrophysics (2012)

1117 Citations

Evolutionary stellar population synthesis with MILES: I. The base models and a new line index system

A. Vazdekis;A. Vazdekis;P. Sánchez-Blázquez;P. Sánchez-Blázquez;J. Falcón-Barroso;J. Falcón-Barroso;A. J. Cenarro;A. J. Cenarro.
Monthly Notices of the Royal Astronomical Society (2010)

947 Citations

An updated MILES stellar library and stellar population models (Research Note)

J. Falcon-Barroso;P. Sanchez-Blazquez;A. Vazdekis;E. Ricciardelli.
Astronomy and Astrophysics (2011)

772 Citations

An updated MILES stellar library and stellar population models

J. Falcón-Barroso;P. Sánchez-Blázquez;A. Vazdekis;E. Ricciardelli.
arXiv: Cosmology and Nongalactic Astrophysics (2011)

733 Citations

The O3N2 and N2 abundance indicators revisited: improved calibrations based on CALIFA and Te-based literature data

R. A. Marino;F. F. Rosales-Ortega;S. F. Sánchez;A. Gil de Paz.
arXiv: Cosmology and Nongalactic Astrophysics (2013)

585 Citations

A characteristic oxygen abundance gradient in galaxy disks unveiled with CALIFA

S. F. Sanchez;F. F. Rosales-Ortega;J. Iglesias-Paramo;M. Molla.
arXiv: Cosmology and Nongalactic Astrophysics (2013)

579 Citations

Evolutionary Stellar Population Synthesis with MILES. Part I: The Base Models and a New Line Index System

A. Vazdekis;P. Sánchez-Blázquez;J. Falcón-Barroso;A. J. Cenarro.
arXiv: Cosmology and Nongalactic Astrophysics (2010)

524 Citations

The O3N2 and N2 abundance indicators revisited: improved calibrations based on CALIFA and T e-based literature data

R. A. Marino;F. F. Rosales-Ortega;F. F. Rosales-Ortega;Sebastian Francisco Sanchez Sanchez;A. Gil De Paz.
Astronomy and Astrophysics (2013)

440 Citations

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